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CONFIRMED EXOPLANET · Sub-Neptune

TOI-3896 b

Orbits Host Star: TOI-3896 · Distance: 592.500 Light-Years (181.653 pc)
Planetary Radius
3.149 R⊕
Planetary Mass
10.100 M⊕
Surface Gravity
1.02 g / g⊕
Equilibrium Temp
966K (+693°C / +1279°F)
Orbital Period
4.377 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.24 / 1.00
Insolation Flux
144.99 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-3896 b is a confirmed sub-neptune exoplanet orbiting the star TOI-3896, located approximately 592.5 light-years (181.65 parsecs) from the Solar System. First announced in 2026 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.149% across the stellar disk), this world measures 3.149 Earth radii (0.28 Jupiter radii) and has a measured mass of 10.1 Earth masses. Combining its mass and radius yields a mean bulk density of 1.78 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1.02 g⊕ (10 m/s²), and an escape velocity of 20 km/s.

In its orbital architecture around TOI-3896, TOI-3896 b completes one full revolution every 4.377 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 966 K (+693°C / +1279°F) and receiving 144.99 S⊕ (~197,329 W/m²), TOI-3896 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-3896 is classified as a stellar host with an effective photospheric temperature of 5,111 K, a radius of 0.7478 R☉, a mass of 0.86 M☉, an estimated bolometric luminosity of 0.342 L☉. From Earth, TOI-3896 shines at apparent V-band magnitude 12.43 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.24 Earth Baseline = 1.00
0.00 Dissimilar 0.50 Mars Scale 0.70 Analog Regime 1.00 Earth

Methodology: Computed using the Schulze-Makuch et al. (2011) weighted metric comparing physical interior (radius, estimated density) and surface thermal regime (escape velocity, equilibrium temperature).

Discovery Facility: Transiting Exoplanet Survey Satellite (TESS) · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name TOI-3896
Spectral Type Unclassified
Effective Temp (Teff) 5,111 K
Stellar Radius 0.7478 R☉
Stellar Mass 0.8600 M☉
Bolometric Luminosity 0.342 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 12.430 · G: 12.233
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 4.377 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 87.7484°
Mean Bulk Density 1.78 g/cm³ (20 km/s vesc)
Insolation Flux 144.9880 S⊕ (~197,329 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 592.500 LY (181.653 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 12h31m43.26s · DEC: +63d54m30.77s (J2000: 187.93024°, 63.90855°)
Target Field: TOI-3896 (J2000 187.93024°, 63.90855°)
Surveys available: Digitized Sky Survey (DSS2 Optical), 2MASS (Near-Infrared), AllWISE (Mid-Infrared) · Field of View: 0.18° (10.8 arcmin)
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